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Table 4
Best-fit planetary radius derived in the different wavelength bins using observations from HARPS, CARMENES-VIS, CARMENES-NIR, and the combination of all instruments.
| λ (nm) | Rp∕R⋆ | Error |
|---|---|---|
| HARPS | ||
| 395.0 | 0.1598 | 0.0025 |
| 445.0 | 0.1614 | 0.0032 |
| 495.0 | 0.1607 | 0.0029 |
| 545.0 | 0.1615 | 0.0032 |
| 575.0 | 0.1623 | 0.0022 |
| 625.0 | 0.1612 | 0.0018 |
| 675.0 | 0.1573 | 0.0036 |
| CARMENES-VIS | ||
| 545.0 | 0.1585 | 0.0022 |
| 575.0 | 0.1622 | 0.0029 |
| 625.0 | 0.1609 | 0.0017 |
| 675.0 | 0.1576 | 0.0029 |
| 725.0 | 0.1574 | 0.0021 |
| 775.0 | 0.1625 | 0.0035 |
| 825.0 | 0.1577 | 0.0047 |
| 875.0 | 0.1587 | 0.0047 |
| 935.0 | 0.1545 | 0.0056 |
| CARMENES-NIR | ||
| 997.5 | 0.1499 | 0.0057 |
| 1067.5 | 0.1507 | 0.0044 |
| 1195.0 | 0.1602 | 0.0060 |
| 1287.5 | 0.1526 | 0.0062 |
| 1550.0 | 0.1507 | 0.0061 |
| 1650.0 | 0.1620 | 0.0071 |
| Combined | ||
| 395.0 | 0.1598 | 0.0025 |
| 445.0 | 0.1614 | 0.0032 |
| 495.0 | 0.1607 | 0.0029 |
| 545.0 | 0.1599 | 0.0029 |
| 575.0 | 0.1622 | 0.0029 |
| 625.0 | 0.1610 | 0.0011 |
| 675.0 | 0.1574 | 0.0021 |
| 725.0 | 0.1574 | 0.0021 |
| 775.0 | 0.1625 | 0.0035 |
| 825.0 | 0.1577 | 0.0047 |
| 875.0 | 0.1587 | 0.0047 |
| 935.0 | 0.1545 | 0.0056 |
| 997.5 | 0.1499 | 0.0057 |
| 1067.5 | 0.1507 | 0.0044 |
| 1195.0 | 0.1602 | 0.0060 |
| 1287.5 | 0.1526 | 0.0062 |
| 1550.0 | 0.1507 | 0.0061 |
| 1650.0 | 0.1620 | 0.0071 |
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